TY - JOUR
T1 - Comparison of heavy-ion transport simulations
T2 - Collision integral with pions and Δ resonances in a box
AU - Ono, Akira
AU - Xu, Jun
AU - Colonna, Maria
AU - Danielewicz, Pawel
AU - Ko, Che Ming
AU - Tsang, Manyee Betty
AU - Wang, Yong Jia
AU - Wolter, Hermann
AU - Zhang, Ying Xun
AU - Chen, Lie Wen
AU - Cozma, Dan
AU - Elfner, Hannah
AU - Feng, Zhao Qing
AU - Ikeno, Natsumi
AU - Li, Bao An
AU - Mallik, Swagata
AU - Nara, Yasushi
AU - Ogawa, Tatsuhiko
AU - Ohnishi, Akira
AU - Oliinychenko, Dmytro
AU - Su, Jun
AU - Song, Taesoo
AU - Zhang, Feng Shou
AU - Zhang, Zhen
N1 - Funding Information:
A. Ono acknowledges support from Japan Society for the Promotion of Science KAKENHI Grants No. JP24105008 and No. JP17K05432. J. Xu was supported by the Major State Basic Research Development Program (973 Program) of China under Contract No. 2015CB856904, and the National Natural Science Foundation of China under Grants No. 11922514 and No. 11421505. M. Colonna acknowledges the support from the European Unions Horizon 2020 research and innovation programme under Grant Agreement No. 654002. P. Danielewicz was supported by the U.S. Department of Energy Office of Science under Grant No. DE-SC0019209. C. M. Ko was supported by the U.S. Department of Energy under Contract No. DE-SC0015266 and the Welch Foundation under Grant No. A-1358. Y. J. Wang was supported by the National Natural Science Foundation of China under Grants No. 11847315, No. 11875125, and No. 11505057. H. H. Wolter was supported by the Universe Cluster of the German Research Foundation (DFG). L. W. Chen was supported by the National Natural Science Foundation of China under Grant No. 11625521. B. A. Li is supported by the U.S. Department of Energy under Award No. DE-SC0013702. T. Ogawa acknowledges support from Japan Society for the Promotion of Science KAKENHI Grant No. JP26790072. D. Oliinychenko was supported by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics, under Contract No. DE-AC02-05CH11231 and received support within the framework of the Beam Energy Scan Theory (BEST) Topical Collaboration. P. Danielewicz, M. B. Tsang, C. M. Ko, and B. A. Li are also supported by the CUSTIPEN (China-U.S. Theory Institute for Physics with Exotic Nuclei) under the U.S. Department of Energy Grant No. DE-SC0009971. The computation by the JAM code was carried out at the HOKUSAI supercomputer system of RIKEN. The authors acknowledge the support by the organizers of the Transport Workshop held in Busan, South Korea, September 14–15, 2018, which was organized for the discussions on the present work and related subjects. The writing committee (consisting of the first nine authors) would like to acknowledge the generous financial support from the director of the Facility for Rare Isotope Beams (FRIB) in hosting writing sessions at the 2017 International Collaboration in Nuclear Theory (ICNT). Writing sessions by J.X., A.O., M.B.T., and Y.X.Z. were also hosted at the Chinese Institute of Atomic Energy (CIAE), with support from CIAE funding and State Administration of Foreign Experts Affairs, No. T170517002. Other writing sessions by A.O., J.X., C.M.K., M.B.T., and Y.X.Z. were hosted at Sun Yat-sen University. The stay of A.O. during the ICNT meeting was supported by National Science Foundation under Grant No. PHY-1430152 (JINA Center for the Evolution of the Elements).
Publisher Copyright:
© 2019 American Physical Society.
PY - 2019/10/30
Y1 - 2019/10/30
N2 - Background: Simulations by transport codes are indispensable for extracting valuable physical information from heavy-ion collisions. Pion observables such as the π-/π+ yield ratio are expected to be sensitive to the symmetry energy at high densities. Purpose: To evaluate, understand, and reduce the uncertainties in transport-code results originating from different approximations in handling the production of Δ resonances and pions. Methods: We compare ten transport codes under controlled conditions for a system confined in a box, with periodic boundary conditions, and initialized with nucleons at saturation density and at a temperature of 60 MeV. The reactions NN↔NΔ and Δ↔Nπ are implemented, but the Pauli blocking and the mean-field potential are deactivated in the present comparison. Thus, these are cascade calculations including pions and Δ resonances. Results are compared to those from the two reference cases of a chemically equilibrated ideal gas mixture and of the rate equation. Results: For the numbers of Δ and π, deviations from the reference values are observed in many codes, and they depend significantly on the size of the time step. These deviations are tied to different ways in ordering the sequence of reactions, such as collisions and decays, that take place in the same time step. Better agreements with the reference values are seen in the reaction rates and the number ratios among the isospin species of Δ and π. Both the reaction rates and the number ratios are, however, affected by the correlations between particle positions, which are absent in the Boltzmann equation, but are induced by the way particle scatterings are treated in many of the transport calculations. The uncertainty in the transport-code predictions of the π-/π+ ratio, after letting the existing Δ resonances decay, is found to be within a few percent for the system initialized at n/p=1.5. Conclusions: The uncertainty in the final π-/π+ ratio in this simplified case of particles in a box is sufficiently small so that it does not strongly impact constraining the high-density symmetry energy from heavy-ion collisions. Most of the sources of uncertainties have been understood, and individual codes may be further improved in future applications. This investigation will be extended in the future to heavy-ion collisions to ensure the problems identified here remain under control.
AB - Background: Simulations by transport codes are indispensable for extracting valuable physical information from heavy-ion collisions. Pion observables such as the π-/π+ yield ratio are expected to be sensitive to the symmetry energy at high densities. Purpose: To evaluate, understand, and reduce the uncertainties in transport-code results originating from different approximations in handling the production of Δ resonances and pions. Methods: We compare ten transport codes under controlled conditions for a system confined in a box, with periodic boundary conditions, and initialized with nucleons at saturation density and at a temperature of 60 MeV. The reactions NN↔NΔ and Δ↔Nπ are implemented, but the Pauli blocking and the mean-field potential are deactivated in the present comparison. Thus, these are cascade calculations including pions and Δ resonances. Results are compared to those from the two reference cases of a chemically equilibrated ideal gas mixture and of the rate equation. Results: For the numbers of Δ and π, deviations from the reference values are observed in many codes, and they depend significantly on the size of the time step. These deviations are tied to different ways in ordering the sequence of reactions, such as collisions and decays, that take place in the same time step. Better agreements with the reference values are seen in the reaction rates and the number ratios among the isospin species of Δ and π. Both the reaction rates and the number ratios are, however, affected by the correlations between particle positions, which are absent in the Boltzmann equation, but are induced by the way particle scatterings are treated in many of the transport calculations. The uncertainty in the transport-code predictions of the π-/π+ ratio, after letting the existing Δ resonances decay, is found to be within a few percent for the system initialized at n/p=1.5. Conclusions: The uncertainty in the final π-/π+ ratio in this simplified case of particles in a box is sufficiently small so that it does not strongly impact constraining the high-density symmetry energy from heavy-ion collisions. Most of the sources of uncertainties have been understood, and individual codes may be further improved in future applications. This investigation will be extended in the future to heavy-ion collisions to ensure the problems identified here remain under control.
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U2 - 10.1103/PhysRevC.100.044617
DO - 10.1103/PhysRevC.100.044617
M3 - Article
AN - SCOPUS:85074943653
SN - 2469-9985
VL - 100
JO - Physical Review C
JF - Physical Review C
IS - 4
M1 - 044617
ER -